. Go Here for Hubble Ultra Deep Field . ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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• The Galaxy Gallery: Messier Objects
• Physics 410/510 Observational Cosmology
• Astronomy HyperText Book

... The Chandra Multiwavelength Project (ChaMP) seeks to understand the nature and evolution of quasars, galaxies, and clusters of galaxies in a large, carefully constructed multi-wavelength survey. ... Recent ChaMP Papers . The Field X-ray AGN Fraction to z=0.7 from the Chandra Multiwavelength Project and the Sloan Digital Sky Survey , Haggard, D., Green, P.J., Anderson, S.F., Constantin, A., Aldcroft, T., Kim, D.-W., Barkhouse, W.A. 2010, ApJ, 723, 1447 (arXiv:1004.1638) . ... 2009, ApJ, 690, 644 . ...

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• SAO Summer Intern Program Projects, 2004
• ChASeM33 Source Catalog
• The Chandra Multiwavelength Project (ChaMP) - Science Goals

... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...

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• Seminars

... RATAN-600 data for the BL Lacertae objects (multi-frequency catalogue, Version 1.0) . GPS radio sources . ... BL Lacertae objects . ... The difference between these objects is the peak frequency of the synchrotron component of their spectral energy distribution (HBLs: high-energy peak, LBLs: low-energy peak, IBLs: intermediate). ... The observations were carried out with the RATAN-600 radio telescope during 2006-2011 at six frequencies: 1.1, 2.3, 4.8, 7.7, 11.2 and 21.7 GHz. ...

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• A 1400-MHz Survey of 1478 Abell Clusters of Galaxies
• A VLA Survey of Rich Clusters of Galaxies I.
• The very metal-poor local dwarf galaxies

Next: Sample Properties Up: Sample Identification Previous: Comments on Individual Sources . Previously known serendipitous sources were selected by cross-correlating WGACAT with a variety of optical and radio catalogs, including the Ver?n-Cetty & Ver?n (1996) and Hewitt & Burbidge (1993) quasar catalogs, the 1 Jy (Stickel et al. 1994) and S4 (Stickel & K?hr 1994) radio catalogs, and the BL Lac catalog of Padovani & Giommi (1995b). ... Details of these 97 objects are given in Table 6. ...

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• ESO - Science in Garching
• ESO - Studying the Cosmological Evolution of Galaxy Clusters with (Sub-)mm
• ESO - Newsletter December 2015

Hide Zen home . ... sncat2sntab.pl - convert old catalog to table sn . ... CREATE TABLE cats ( id integer PRIMARY KEY, name text ); -- a list of properties of galaxy CREATE TABLE properties ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy _property ( gid integer REFERENCES galaxy (id), pid integer REFERENCES properties(id), value float, UNIQUE( gid ,pid) ); CREATE t=# select * from galaxy; id | ...

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• APOD: September 29, 1998 - A Peculiar Cluster of Galaxies
• Zen: pg80-pr-en

... Staff . ... Galaxies, AGN, Cosmology . ... A new survey of X-ray clusters of galaxies with the Swift-X-ray Telescope . ... In this framework, an international collaboration between INAF-OAA, INAF-Brera, INAF-OATs, the University for Science and Technology of China-Hefei, the University of Ferrara, and the University of Massachusetts-Amherst, is undertaking a new cluster survey using an X-ray facility that was never exploited before for this goal: the X-ray Telescope (XRT) onboard the Swift satellite...

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• SECCO1: an "almost-dark" dwarf galaxy
• The puzzling core of the Phoenix cluster: deep X-ray observations
• GIANO opens a new window on stellar and planetary astrophysics

... The basics · · · · Source galaxy at Observed image at Instead of I(), we see I'[()] We care about the Jacobian: = convergence; = shear Definitions = projected surface ... (axisymmetric) Definitions = projected surface density contrast (axisymmetric) = shear (comoving) Sloan Digital Sky Survey ( SDSS ) Imaging, spectroscopy over ~ 1/4 of the sky Imaging in 5 passbands (ugriz) (from http://www. sdss .org/) Our approach: Reglens Lenses: SDSS spectroscopic sample (~4x105 ...

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• Lou Strolger's Page
• Life Cycles of Radio Galaxies - Final Program
• Our group

ATCA Legacy Project Expression of Interest: WALLABY@ATCA Title: Au t h o r s : Point of contact: WALLABY@ATCA L i s t e r S t a v e l e y - S m i t h , B Д r b e l Ko r i b a l s k i , P a o l o S e r r a , To b i a s We s t m e i e r ( o n b e h a l f o f t h e WA L L A B Y t e a m ) To b i a s We s t m e i e r Scientific Aims The aims of the Widefield ASKAP L-band Legacy All-sky Blind surveY ( ... WALLABY@ATCA would only observe a small fraction of `interesting' WALLABY discover ies. ...

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• projects
• HIPASS Bright Galaxy Catalog
• Evolutionary Paths in Galaxy Morphology

Magnetic Fields around Radio Galaxies Robert Laing (ESO) Laing et al. ... 2008) Negligible depolarization and 2 rotation Almost all Faraday effects must be due to foreground material How to fit depolarization caused by foreground Faraday rotation Complex polarization Rotation measure Integrate over a beam Observed RM for 0 2 rotation and depolarization Faraday rotation and depolarization 5.5 arcsec FWHM Faraday effects at high resolution FWHM = 1.5 ...

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• Astrophysics Group Available research projects/areas
• Galaxy Evolution: Regulation of the ISM and Star Formation
• Galaxy Evolution: The origin and evoltuion of radio sources

Other databases on optical properties of scatterers as far as we know are as follows (we shall be thankful to anyone who will provide us with more information!) ... Resources containing light scattering codes to calculate the optical properties of different scatterers have been mentioned in the corresponding section . Some bibliographies on light scattering including the questions of the optical properties have been referred to in the corresponding section . ...

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• Vladimir P. Reshetnikov's Home Page
• Database of Optical Properties -- Level: subsubpage
• Database of Optical Properties -- Level: database

... The study of the Large-scale structure of the Universe and measurements of the Dark Energy equation of state; The exploration of the growth and cosmological evolution of supermassive Black holes in the Universe. ... In course of the all sky survey SRG will discover about 100 000 galaxy clusters and 3 million AGNs. Galaxy clusters are the largest gravitationally bounded objects in the Universe and are best explored through the study of X-ray emission from the hot intergalactic gas. ... 2016 IKI RAN ...

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• High Energy Astrophysics Department at IKI RAN
• z90-program
• Second Spectrum-RG/eROSITA Conference

Neutral Hydrogen and Star Formation in the Coma-A1367 Supercluster. Luca Cortese School of Physics & Astronomy ­ Cardiff University Outline of the Project GOAL: Gain additional insights on the mechanisms and timescales which regulates the migration of galaxies (L>109 L ) from the blue to the red sequence by combining UV and HI. ... By combining HI and UV data we can select galaxies at different stages of their transition between the blue and the red sequence! ... 2005) But...the TIR/FUV vs. ...

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• REU Science Area
• NAIC-NRAO Single Dish Summer School 2005 NAIC-NRAO Single Dish Summer School
• VLBI at Arecibo Observatory

... Spectrum-RG is joint project of Russian Federal Space Agency (Roscosmos) and German Space Agency (DLR) of X-ray astrophysical observatory. Its main aim is to make all-sky survey in the X-ray (0.5-11 keV) band in order to find all massive clusters of galaxies in the Universe, millions of active galactic nuclei, including obscured ones and hundreds of thousands of Galactic X-ray sources. ... eRosita (Germany) X-ray grazing-incident mirror telescope, consisting of 432 mirrors combined in 7 modules. ...

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• "Exploration" as a Classroom Resource

Title: A New Model of the Gravitational Lens 0957+561 and a Limit on the Hubble Constant . Authors: Norman A. Grogin , Ramesh Narayan (Harvard Univ.) ... Title: ROSAT/PSPC observation of the distant cluster CL0939+472 . ... Title: Interaction in the Bimodal Galaxy Cluster A3528 . ... Title: Cosmological Implications of Galaxy Cluster Evolution . ... Title: Galaxy Cluster Virial Masses and Omega . ... Matches 201 to 222 from a total of 222 matches for the search pattern galaxy cluster . ...

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• Radio galaxies
• astro-ph authors/title/abstract search for 'galaxy merging' all years
• Relative literature to radio galaxy study

... The search for distant objects which can be both galaxies and quasars is one of the most important problems of observational astrphysics, because it allows one to determine cosmological parameters connected with the time of appearence and evolution of stellar systems, large scale structure of the Universe. ... Radio galaxies are important objects to be studied because they are sources of infrared-optical-ultraviolet continuum, emission lines and continual radio emission. ...

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• SCORPIO-2 project: publications
• Radio sources identfification
• RESEARCH PROBLEMS of the LRS

Stellarium 0.12.3 . ... core . ... 198 љ void artDisplayedChanged( const bool displayed) const ; . ... 202 љ void boundariesDisplayedChanged( const bool displayed) const ; . ... 204 љ void isolateSelectedChanged( const bool isolate) const ; . ... 206 љ void linesDisplayedChanged( const bool displayed) const ; . ... 208 љ void namesDisplayedChanged( const bool displayed) const ; . ... 239 љ void loadLinesAndArt( const QString& fileName, const QString& artfileName, const QString& cultureName); . ...

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• Stellarium: core/modules/GridLinesMgr.hpp Source File
• Stellarium: /home/aw/devel/stellarium/trunk/plugins/Oculars/src/CCD.hpp Source
• Stellarium: core/modules/LandscapeMgr.hpp Source File

... A radio galaxy is a galaxy that emits an unusually big amount of energy at radio wavelengths. ... Inside of each galaxy with an active nucleus (radio galaxies are among them) there must be a system of a "central machine" responsible for the colossal amount of the emitted energy from radio to gamma ranges. ... Sometimes a radio source in an active galaxy may flare again if the needed conditions appear (a new portion of matter would fall into the furnace of the "central machine"). ...

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• Detection of Radio Transients and Variable Radio Sources Using the Archive Data
• Galaxy sector, archive 2012
• articles_flera_en

... Data Analysis SAS News What is SAS? ... Archive, Pipeline & Catalogues XMM-Newton Science Archive Pipeline Processing System Observation Data Status Time Correlation Fix Serendipitous Source Catalogue OM Serendipitous Source Catalogue Slew Survey Catalogue Latest Slew Results Browsing Interface for RGS Data Live Radiation Monitor Plots Radiation Monitor Files . ... About XMM-Newton Image Gallery XMM-Newton Technical Details XMM-Newton SOC Overview XMM-Newton 10th Anniversary . ...

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• XMM Deep Survey Simulations
• XMM-Newton Trainee Project 2005
• EPIC source list.

... astro-ph . ... Statistical Characterization of the Chandra Source Catalog . ... The first release of the Chandra Source Catalog (CSC) contains ~95,000 X-ray sources in a total area of ~0.75% of the entire sky, using data from ~3,900 separate ACIS observations of a multitude of different types of X-ray sources. ... In addition to these traditional catalog elements, for each X-ray source the CSC includes an extensive set of file-based data products that can be manipulated interactively. ...

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• SAI Virtual Observatory Project - About